A numerical study on climates of synchronously rotating terrestrial planets

在这项研究中，对同步旋转行星上的湿大气结构进行了参数实验，并开发了现实模拟所需的模式基础设施。不同行星自转速度下的参数实验表明，存在南北不对称振荡状态，并存在多重平衡。各种太阳常数的参数实验表明，随着行星自转速度的变化，出现温室失控状态的太阳常数的值约为100W/m^2。此外，还开发了氢气氛的辐射方案和数据输入输出库。

In this study, parameter experiments on structures of moist atmospheres on synchronously rotating planets are performed, and model infrastructure needed for realistic simulations are developed. Parameter experiment with various planetary rotation rate show existence of oscillating north-south asymmetric states and occurence of multiple equilibrium. Parameter experiment with various solar constant show that the value of solar constant at which the runaway greenhouse states occur changes about 100W/m^2 according to the value of planetary rotation rate. Moreover, radiation scheme for hydrogen atmospheres and a data input/output library are developed.